版权说明 操作指南
首页 > 成果 > 详情

Quark matter at finite temperature under strong magnetic fields within Nambu-Jona-Lasinio model

认领
导出
下载 Link by DOI
反馈
分享
QQ微信 微博
成果类型:
期刊论文
作者:
Chu, Peng-Cheng*;Zhou, Yi;Chen, Chang*;Li, Xiao-Hua*;Ma, Hong-Yang*
通讯作者:
Chu, Peng-Cheng;Chen, Chang;Ma, Hong-Yang;Li, Xiao-Hua
作者机构:
[Chu, Peng-Cheng] Qingdao Technol Univ, Sch Sci, Inst Theoret Phys, Qingdao 266000, Peoples R China.
[Chu, Peng-Cheng; Chu, PC; Chen, Chang] Qingdao Technol Univ, Quantum Phys Lab, Qingdao 266000, Peoples R China.
[Zhou, Yi] Qingdao Univ Sci & Technol, Sch Math & Phys, Qingdao 266000, Peoples R China.
[Chen, Chang; Ma, Hong-Yang] Qingdao Technol Univ, Sch Sci, Qingdao 266000, Peoples R China.
[Li, Xiao-Hua] Univ South China, Sch Nucl Sci & Technol, Hengyang 421001, Peoples R China.
通讯机构:
[Chu, Peng-Cheng; Chu, PC; Chen, C; Ma, HY] Q
[Li, Xiao-Hua] U
Qingdao Technol Univ, Sch Sci, Inst Theoret Phys, Qingdao 266000, Peoples R China.
Qingdao Technol Univ, Quantum Phys Lab, Qingdao 266000, Peoples R China.
Qingdao Technol Univ, Sch Sci, Qingdao 266000, Peoples R China.
语种:
英文
关键词:
quark matter;symmetry energy;compact stars
期刊:
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS
ISSN:
0954-3899
年:
2020
卷:
47
期:
8
页码:
085201
基金类别:
NSFCNational Natural Science Foundation of China [11975132, 11505100, 11804179, 61502262, 11205083, 41702322, 61772295]; Natural Science Foundation of Shandong, ChinaNatural Science Foundation of Shandong Province [ZR2019YQ01, ZR2019PA018, ZR2015AQ007, ZR2016DB01]; Research Foundation of Education Bureau of Hunan Province, China [15A159]; Natural Science Foundation of Hunan Province, ChinaNatural Science Foundation of Hunan Province [2015JJ3103]; Shandong Provincial Keypoint Research and Invention Program, China [2017GSF216010]
机构署名:
本校为通讯机构
院系归属:
机械工程学院
核科学技术学院
摘要:
The quark matter symmetry free energy and the thermodynamical properties of strange quark matter (SQM) in strong magnetic fields and non-zero temperature cases are discussed in this work within Nambu–Jona-Lasinio (NJL) model by considering two kinds of vector interactions. The properties of the proto-quark stars (PQSs) are also studied by introducing a density-dependent magnetic field strength distribution and assuming two 'extreme' magnetic orientation cases inside the quark stars (QSs). The results indicate that the strength and orientation ...

反馈

验证码:
看不清楚,换一个
确定
取消

成果认领

标题:
用户 作者 通讯作者
请选择
请选择
确定
取消

提示

该栏目需要登录且有访问权限才可以访问

如果您有访问权限,请直接 登录访问

如果您没有访问权限,请联系管理员申请开通

管理员联系邮箱:yun@hnwdkj.com